Role of anisotropic confining potential and elliptical driving in dynamics of a Ge hole qubit.

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Tác giả: Bashab Dey, John Schliemann

Ngôn ngữ: eng

Ký hiệu phân loại:

Thông tin xuất bản: England : Journal of physics. Condensed matter : an Institute of Physics journal , 2025

Mô tả vật lý:

Bộ sưu tập: NCBI

ID: 474738

 The squeezing of a Ge planar quantum dot enhances the Rabi frequency of electric dipole spin
 resonance by several orders of magnitude due to a strong Direct Rashba spin-orbit interaction (DR-
 SOI) in such geometries [Phys. Rev. B 104, 115425 (2021)]. We investigate the geometric effect
 of an elliptical (squeezed) confinement and its interplay with the polarization of driving field in
 determining the Rabi frequency of a heavy-hole qubit in a planar Ge quantum dot. To calculate
 the Rabi frequency, we consider only the p-linear SOIs viz. electron-like Rashba, hole-like Rashba
 and hole-like Dresselhaus which are claimed to be the dominant ones by recent studies on planar
 Ge heterostructures. We derive approximate analytical expressions of the Rabi frequency using a
 Schrieffer-Wolff transformation for small SOI and driving strengths. Firstly, for an out-of-plane
 magnetic field with magnitude B, we get an operating region with respect to B, squeezing and
 polarization parameters where the qubit can be operated to obtain 'clean' Rabi flips. On and
 close to the boundaries of the region, the higher orbital levels strongly interfere with the two-level
 qubit subspace and destroy the Rabi oscillations, thereby putting a limitation on squeezing of the
 confinement. The Rabi frequency shows different behaviour for electron-like and hole-like Rashba
 SOIs. It vanishes for right (left) circular polarization in presence of purely electron-like (hole-
 like) Rashba SOI in a circular confinement. For both in- and out-of-plane magnetic fields, higher
 Rabi frequencies are achieved for squeezed configurations when the ellipses of polarization and the
 confinement equipotential have their major axes aligned but with different eccentricities. We also
 deduce a simple formula to calculate the effective heavy hole mass by measuring the Rabi frequencies
 using this setup.
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